Search results for "IDENTIFICATION"

showing 10 items of 1600 documents

Endcap Disc DIRC for PANDA at FAIR

2018

The Endcap Disc DIRC (EDD) has been developed to provide an excellent particle identification in the future PANDA experiment by separating pions and kaons up to a momentum of 4 GeV/c with a separation power of 3 s.d.. The detector is placed in the forward endcap of the PANDA target spectrometer. It consists of a fused silica plate and focusing elements placed at the outer rim, which focus the Cherenkov light on the photo cathodes of the attached MCP-PMTs. A compact and fast readout of the signals is realized with special ASICs. The performance has been studied and validated with different prototype setups in various testbeam facilities.

PhysicsSpectrometerPhysics::Instrumentation and Detectorsbusiness.industryCherenkov detectorDetectorParticle identificationlaw.inventionOpticslawHigh Energy Physics::ExperimentNuclear ExperimentbusinessCherenkov radiation
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Three-prong τ decays with charged kaons

1998

Final states with charged kaons in three-prong τ decays are studied by exploiting the particle identification from the dE/dx measurement. The results are based on a sample of about 1.6 × 105 detected τ pairs collected with the ALEPH detector between 1991 and 1995 around the Z peak. The following branching ratios have been measured: B(τ- → K−K+π−ντ) = (1.63 ± 0.21 ± 0.17) × 10−3, B(τ− → K−π+π−ντ) = (2.14 ± 0.37 ± 0.29) × 10−3, B(τ− → K−K+π−π0ντ) = (0.75 ± 0.29 ± 0.15) × 10−3, and B(τ− → K−π+π−π0ντ) = (0.61 ± 0.39 ± 0.18) × 10−3. The first two measurements are more precise than the current world averages, while the last two channels are investigated for the first time. The 95% C.L. upper limi…

PhysicsSystematic errorTime projection chamberPhysics and Astronomy (miscellaneous)010308 nuclear & particles physicsBranching fractionHigh Energy Physics::PhenomenologySettore FIS/01 - Fisica SperimentaleVECTOR01 natural sciencesMESONSParticle identificationPHYSICS0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]High Energy Physics::ExperimentAtomic physics010306 general physicsEngineering (miscellaneous)Particle Physics - Experiment
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Pseudospin Symmetry and Microscopic Origin of Shape Coexistence in the Ni78 Region: A Hint from Lifetime Measurements

2018

Lifetime measurements of excited states of the light N = 52 isotones 88 Kr , 86 Se , and 84 Ge have been performed, using the recoil distance Doppler shift method and VAMOS and AGATA spectrometers for particle identification and gamma spectroscopy, respectively. The reduced electric quadrupole transition probabilities B ( E 2 ; 2 + → 0 + ) and B ( E 2 ; 4 + → 2 + ) were obtained for the first time for the hard-to-reach 84 Ge . While the B ( E 2 ; 2 + → 0 + ) values of 88 Kr , 86 Se saturate the maximum quadrupole collectivity offered by the natural valence ( 3 s , 2 d , 1 g 7 / 2 , 1 h 11 / 2 ) space of an inert 78 Ni core, the value obtained for 84 Ge largely exceeds it, suggesting that sh…

PhysicsValence (chemistry)Proton010308 nuclear & particles physicsGeneral Physics and Astronomy01 natural sciencesParticle identificationRecoilExcited state0103 physical sciencesQuadrupoleNeutronAGATAAtomic physics010306 general physicsPhysical Review Letters
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Rule-guided identification of cosmic-ray patterns in PLASTEX

1992

Some techniques devised in the computer science fields of pattern recognition and expert systems are being applied to the interpretation of EAS responses in the PLASTEX experiment. An attempt is made to codity in a set of rules the expertise of trained researchers who are able to recognize and classify different hit patterns even in the presence of noisy background, and in spite of imperfections in the detector response. The patterns expected to be useful include, but are not limited to, track patterns. The software described here, as a progress report, automatically finds patterns corresponding to isolated tracks, and patterns composed of tracks that connect with each other in a layer of d…

Physicsbusiness.industryDetectorProbabilistic logiccomputer.software_genreExpert systemSet (abstract data type)Identification (information)SoftwareOpticsPattern recognition (psychology)Extensive air showersCosmic-raysData pre-processingbusinessComputation techniquesPACS 94.40.MyAlgorithmcomputer
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Chandra Observation of the Persistent Emission from the Dipping Source XB 1916-053

2006

We present the results of a 50 ks long Chandra observation of the dipping source XB 1916-053. During the observation two X-ray bursts occurred and the dips were not present at each orbital period. From the zero-order image we estimate the precise X-ray coordinates of the source with a 90% uncertainty of 0.6''. In this work we focus on the spectral study of discrete absorption features, during the persistent emission, using the High Energy Transmission Grating Spectrometer on board the Chandra satellite. We detect, for the first time in the 1st-order spectra of XB 1916-053, absorption lines associated to Ne X, Mg XII, Si XIV, and S XVI, and confirm the presence of the Fe XXV and Fe XXVI abso…

Physicsline : formationAbsorption spectroscopySpectrometerAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysicsOrbital periodstars : neutronSpectral linestars : individual (XB 1916-053)Neutron starline : identificationSpace and Planetary Scienceformation; line : identification; stars : individual (XB 1916-053); stars : neutron; X-rays : binaries; X-rays : general [line]Absorption (electromagnetic radiation)X-rays : binarieDiffraction gratingLine (formation)X-rays : general
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A Complex Environment around Circinus X-1

2007

We present the results of an archival 54 ks long Chandra observation of the peculiar source Cir X-1 during the phase passage 0.223-0.261. We focus on the study of detected emission and absorption features using the HETGS. A comparative analysis of X-ray spectra, selected at different flux levels of the source, allows us to distinguish between a very hard state, at a low count rate, and a brighter, softer, highly absorbed spectrum during episodes of flaring activity. The spectrum of the hard state clearly shows emission lines of highly ionized elements, while, during the flaring state, the spectrum also shows strong resonant absorption lines. The most intense and interesting feature in this …

Physicsline : formationAccretion (meteorology)Astrophysics::High Energy Astrophysical PhenomenaX-ray binaryAstronomy and AstrophysicsAstrophysicsSpectral lineline : identificationAbsorption edgeSpace and Planetary ScienceIonizationCircinusEmission spectrumstars : individual (Circinus X-1)formation; line : identification; stars : individual (Circinus X-1); X-rays : binaries; X-rays : general [line]Atomic physicsAbsorption (electromagnetic radiation)X-rays : binarieX-rays : general
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Laboratory astrophysics survey of key x-ray diagnostic lines using a microcalorimeter on an electron beam ion trap

2000

Cosmic plasma conditions created in an electron beam ion trap (EBIT) make it possible to simulate the dependencies of key diagnostic X-ray lines on density, temperature, and excitation conditions that exist in astrophysical sources. We used a microcalorimeter for such laboratory astrophysics studies because it has a resolving power ≈1000, quantum efficiency approaching 100%, and a bandwidth that spans the X-ray energies from 0.2 keV to 10 keV. Our microcalorimeter, coupled with an X-ray optic to increase the effective solid angle, provides a significant new capability for laboratory astrophysics measurements. Broadband spectra obtained from the National Institute of Standards and Technology…

Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical Phenomenachemistry.chemical_elementFizikai tudományokAstrophysicsSpectral lineNeonTermészettudományokAtomic processeIonizationPhysics::Atomic PhysicsAtomic dataNuclear and High Energy PhysicPhysicsArgonKryptonAstronomy and AstrophysicsLine: IdentificationPlasmaX-rays: GeneralchemistrySpace and Planetary ScienceAstrophysical plasmaMethods: Laboratory plasmaAtomic physicsElectron beam ion trap
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A method for detection of muon induced electromagnetic showers with the ANTARES detector

2012

The primary aim of ANTARES is neutrino astronomy with upward going muons created in charged current muon neutrino interactions in the detector and its surroundings. Downward going muons are background for neutrino searches. These muons are the decay products of cosmic-ray collisions in the Earths atmosphere far above the detector. This paper presents a method to identify and count electromagnetic showers induced along atmospheric muon tracks with the ANTARES detector. The method is applied to both cosmic muon data and simulations and its applicability to the reconstruction of muon event energies is demonstrated. © 2012 Elsevier B.V. All rights reserved.

Physics::Instrumentation and DetectorsAtmospheric muonsDecay productsNeutrino telescopeElectromagnetic shower identification01 natural sciences7. Clean energyneutrino telescope electromagnetic shower identification high energy muons energy reconstruction; high energy muons; neutrino telescope; electromagnetic shower identification; energy reconstructionMuon neutrinoNEUTRINO TELESCOPE010303 astronomy & astrophysicsInstrumentationEnergy reconstructionPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph][SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]DetectorAstrophysics::Instrumentation and Methods for AstrophysicsDetectorsHigh energy muonNeutrino detectorMuon colliderNeutrino astronomyFísica nuclearNeutrinoNeutrino telescope; Energy reconstruction; High energy muonsAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaFLUXNuclear and High Energy PhysicsParticle physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Charged current[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayMuon neutrinoNuclear physicsElectromagnetism0103 physical sciencesHigh energy physicsneutrino telescope electromagnetic shower identification high energy muons energy reconstructionInstrumentation and Methods for Astrophysics (astro-ph.IM)MuonANTARES010308 nuclear & particles physicsCharged particles[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]FISICA APLICADATEVPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNeutrino astronomyNeutrino telescopesElectro-magnetic showersHigh energy muons
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Combined performance studies for electrons at the 2004 ATLAS combined test-beam

2010

In 2004 at the ATLAS (A Toroidal LHC ApparatuS) combined test beam, one slice of the ATLAS barrel detector (including an Inner Detector set-up and the Liquid Argon calorimeter) was exposed to particles from the H8 SPS beam line at CERN. It was the first occasion to test the combined electron performance of ATLAS. This paper presents results obtained for the momentum measurement p with the Inner Detector and for the performance of the electron measurement with the LAr calorimeter (energy E linearity and resolution) in the presence of a magnetic field in the Inner Detector for momenta ranging from 20 GeV/c to 100 GeV/c. Furthermore the particle identification capabilities of the Transition Ra…

Physics::Instrumentation and DetectorsCiências Naturais::Ciências Físicas:Ciências Físicas [Ciências Naturais]Transition radiation detectorsElectronsddc:500.201 natural sciencesParticle identificationNuclear physicsCalorimetersAtlas (anatomy)Particle tracking detectors0103 physical sciencesmedicine[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Detectors and Experimental Techniques010306 general physicsNuclear ExperimentInstrumentationDetectors de radiacióMathematical PhysicsPhysicsLarge Hadron ColliderScience & Technology010308 nuclear & particles physicsLarge detector systems for particle and astroparticle physicsDetectorCalorimetermedicine.anatomical_structureTransition radiationBeamlineHigh Energy Physics::ExperimentBeam (structure)
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Machine Learning Identification of Pro-arrhythmic Structures in Cardiac Fibrosis

2021

Cardiac fibrosis and other scarring of the heart, arising from conditions ranging from myocardial infarction to ageing, promotes dangerous arrhythmias by blocking the healthy propagation of cardiac excitation. Owing to the complexity of the dynamics of electrical signalling in the heart, however, the connection between different arrangements of blockage and various arrhythmic consequences remains poorly understood. Where a mechanism defies traditional understanding, machine learning can be invaluable for enabling accurate prediction of quantities of interest (measures of arrhythmic risk) in terms of predictor variables (such as the arrangement or pattern of obstructive scarring). In this st…

PhysiologyCardiac fibrosisStimulus (physiology)arrhythmiaMachine learningcomputer.software_genreunidirectional blockFibrosisPhysiology (medical)QP1-981MedicineMyocardial infarctionOriginal ResearchArtificial neural networkbusiness.industryCardiac electrophysiologyMechanism (biology)fibrosisneural networksmedicine.diseaseIdentification (information)machine learningmonodomain modelre-entryArtificial intelligencebusinesscardiac electrophysiologycomputerFrontiers in Physiology
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